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Gaussian Fields and Percolation Dmitry Beliaev Mathematical - PowerPoint PPT Presentation

Gaussian Fields and Percolation Dmitry Beliaev Mathematical Institute University of Oxford RANDOM WAVES IN OXFORD 18 June 2018 Berrys conjecture In 1977 M. Berry conjectured that high energy eigenfunctions in the chaotic case have


  1. Gaussian Fields and Percolation Dmitry Beliaev Mathematical Institute University of Oxford RANDOM WAVES IN OXFORD 18 June 2018

  2. Berry’s conjecture In 1977 M. Berry conjectured that high energy eigenfunctions in the chaotic case have statistically the same behaviour as random plane waves. (Figures from Bogomolny-Schmit paper) Figure: Nodal domains of an eigenfunction (left) of a stadium and of a random plane wave (right)

  3. Random Plane Wave Two ways to (informally) think of the random plane wave A “random” or “typical” solution of Helmholtz equation ∆ f + k 2 f = 0 A random superposition of all possible plane waves with the same frequency k The second approach leads to a naive definition that it is the limit of   n � e k ( θ j , z )+ φ j Ψ n ( z ) = Re   j =1 where θ j are uniform random directions and φ j are random phases.

  4. Gaussian functions and fields Two ways to define Gaussian random functions Random series φ i orthonormal basis in some Hilbert space H � Ψ = a i φ i , a i i . i . d . N (0 , 1) Gaussian field Ψ( x ) is a collection of jointly Gaussian random variables indexed by x . Could be defined by its covariance function K ( x , y ) = E [Ψ( x )Ψ( y )]. Mostly interested in stationary case K ( x , y ) = K ( x − y ). Covariance function � K ( x , y ) = φ i ( x ) φ i ( y )

  5. Stationary Gaussian functions Hilbert space H with a reproducing kernel K ( x , y ). Take any orthonormal basis φ i and construct f = � a i φ i . The result is not in H but independent of the basis. This is a Gaussian field with covariance kernel K ( x , y ). If K ( x , y ) = K ( x − y ) then K is a positive definite function and its Fourier transform is a positive measure ρ . It is called the spectral measure. Properties of f , H , K , and ρ are closely related. In particular, smoothness of K at zero or finite moments of ρ imply smoothness of f .

  6. Random Plane Wave s ( T ) – the Hilbert space of L 2 functions on the unit Consider L 2 circle that satisfy symmetry condition φ ( − z ) = φ ( z ). We define H to be inverse 2d Fourier transform of L 2 s with scalar product inherited from L 2 . This space consist of real analytic functions satisfying Helmholtz equation. Standard basis in L 2 ( T ) is e in θ . This leads to f ( z ) = f ( re i θ ) = � C n J | n | ( r ) e in θ where C n = C − n are independent Gaussian random variables and J n are Bessel functions. The covariant kernel is J 0 ( | z | ) and the spectral measure is d θ/ 2 π .

  7. Related Fields: Random Spherical Harmonic Consider H n the space of all spherical harmonic of degree n with L 2 norm. This is 2 n + 1 dimensional space. A Gaussian vector g n in this space is the random spherical harmonic. Note: H n is an eigenspace of spherical Laplacian with eigenvalue n ( n + 1). Covariance kernel E [ g ( x ) g ( y )] = P n (cos( θ ( x , y ))) where P n is the Legendre polynomial of degree n normalized by P n (1) = 1 and θ ( x , y ) is the angle between x and y (i.e. spherical distance).

  8. Scaling Limit of Random Spherical Harmonics Theorem (Zelditch) Random plane wave is the scaling limit of random spherical harmonic Figure: Nodal lines of a random plane wave and of a random spherical harmonic

  9. Universality of Random Plane Waves Let ( M , g ) be a compact Riemannian manifold, φ i o.n.b. in L 2 ( M ) of eigenfunctions ∆ φ i + λ 2 i φ i = 0 , λ i ≤ λ i +1 Band-limited function � f n ( x ) = c i φ i ( x ) n 2 − n ≤ i ≤ n 2 Scaling limit on the tangent plane: for x 0 ∈ M define F n ( x ) = f n (exp x 0 ( x / n )) where exp x 0 : T x 0 M → M is the exponential map. Then F n converges to the random plane wave as n → ∞ .

  10. Deterministic Results Some universal estimates are known for eigenfunctions of Laplacian. Theorem Nodal set for random plane wave forms a c /λ -net where c is an absolute constant. Nodal set for spherical harmonic forms a c / n-net. Theorem Every nodal component contains a disc of radius c /λ (or c / n) where c is an absolute constant.

  11. Length of Nodal Lines Theorem There is a constant c such that for every spherical harmonic g n of degree n such that n c < L ( g n ) < cn where L ( g n ) is the length of nodal set. Yau conjecture: For a compact C ∞ smooth Riemannian manifold M there is c > 0 such that for every eigenfunction ∆ φ + λ 2 φ = 0 λ/ c ≤ H n − 1 ( φ = 0) ≤ c λ In dimension n = 2 lower bound by Br¨ uning (1978). For n > 2 in real-analytic case by Donnelly-Fefferman (1988), the lower bound in C ∞ case by Logunov (2016).

  12. Nodal Lines of Gaussian Spherical Harmonic Theorem (B´ erard, 1985) For Gaussian spherical harmonic g n of degree n √ √ E L ( g n ) = π 2 λ n = 2 π n + O (1) With more careful analysis of Kac-Rice formula it is possible to compute variance Theorem (Wigman, 2009) For Gaussian spherical harmonic g n of degree n Var L ( g n ) = 1 32 ln( n ) + O (1)

  13. Number of Nodal Domains In the deterministic case Courant’s theorem gives that the number of nodal domains N ( g n ) < n 2 . In 1956 Pleijel improved the upper bound to 0 . 69 n 2 . For n > 2 Lewy constructed spherical harmonic with two or three nodal domains, so there is no non-trivial deterministic lower bound. The main problem: this is a non-local quantity. Theorem (Nazarov and Sodin, 2007) Let g n be Gaussian spherical harmonic of degree n. Then there is a positive constant a such that �� � N ( g n ) � ≤ C ( ǫ ) e − c ( ǫ ) n � � − a � > ǫ P � � n 2 � where C ( ǫ ) and c ( ǫ ) are positive constant depending on ǫ only.

  14. Nodal Domains All positive nodal domains of a random plane wave. Picture by T. Sharpe.

  15. Nodal Domains All negative nodal domains of a random plane wave. Picture by T. Sharpe.

  16. Critical Square Lattice Bond Percolation Each edge of the lattice is preserved with probability p c = 1 / 2. If an edge is preserved, then the dual edge is removed and vice versa. Primal and dual clusters create an loop model of interfaces.

  17. Critical Square Lattice Bond Percolation Each edge of the lattice is preserved with probability p c = 1 / 2. If an edge is preserved, then the dual edge is removed and vice versa. Primal and dual clusters create an loop model of interfaces.

  18. Critical Square Lattice Bond Percolation Each edge of the lattice is preserved with probability p c = 1 / 2. If an edge is preserved, then the dual edge is removed and vice versa. Primal and dual clusters create an loop model of interfaces.

  19. Bogomolny-Schmit Percolation Model They proposed think that the nodal lines form a perturbed square lattice Picture from Bogomolny-Schmit paper.

  20. Bogomolny-Schmit Percolation Model Using this analogy we can think of the nodal domains as percolation clusters on the square lattice. This leads to the conjecture that √ E ( N ( f ) , Ω) = Area (Ω)3 3 − 5 4 π 2

  21. Off-critical Percolation Off-critical percolation is a model for excursion and level sets Figure: Excursion sets for levels 0 (nodal domains) and level 0 . 1

  22. Off-critical Percolation Off-critical percolation is a model for excursion and level sets Figure: Excursion sets for levels 0 (nodal domains) and level 0 . 1

  23. Is It Really True? Numerical results (Nastasescu (2011), Konrad (2012), B.-Kereta (2013)) show that the number of nodal domains per unit area is 0 . 0589 instead of 0 . 0624 predicted by Bogomolny-Schmit. Number of clusters per vertex is a non-universal quantity in percolation, it is lattice dependent. Global properties should be universal i.e. lattice independent. Numerical evidence that many global ‘universal’ observables (crossing probabilities, decay rate for the area of nodal domains, one-arm exponent) match percolation predictions.

  24. Universality Class This seems to be a rather universal phenomenon. For a wide class of smooth stationary fields their nodal domains are in the same universality class as critical percolation. Assumptions: Smooth (nodal lines are nice curves) Stationary (percolation is almost stationary) Isotropic or symmetric enough (uniform conformal structure) Weakly correlated (percolation is local)

  25. A Good Example Bargmann-Fock function 1 2 e −| x | 2 / 2 � 1 x j √ i ! j ! x i f ( x ) = a i , j Covariance kernel K ( x , y ) = e −| x − y | 2 / 2

  26. A Good Example Bargmann-Fock function 1 2 e −| x | 2 / 2 � 1 x j √ i ! j ! x i f ( x ) = a i , j Covariance kernel K ( x , y ) = e −| x − y | 2 / 2

  27. A Good Example Bargmann-Fock function 1 2 e −| x | 2 / 2 � 1 x j √ i ! j ! x i f ( x ) = a i , j Covariance kernel K ( x , y ) = e −| x − y | 2 / 2

  28. A Bad Example White noise on the square lattice Nodal domains are exactly Bernoulli site percolation clusters with p = 1 / 2 which is not critical.

  29. A Bad Example White noise on the square lattice Nodal domains are exactly Bernoulli site percolation clusters with p = 1 / 2 which is not critical.

  30. An Ugly Example Gradient flow percolation model. Nodal domains could be modelled by a lattice model. Not clear how to analyse.

  31. An Ugly Example Gradient flow percolation model. Nodal domains could be modelled by a lattice model. Not clear how to analyse.

  32. An Ugly Example Gradient flow percolation model. Nodal domains could be modelled by a lattice model. Not clear how to analyse.

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